Astrophysical: Methods

  • Publication
    Thermal emission spectra of the ultra-hot Jupiter WASP-33 b
    Observations of exoplanetary atmospheres provide critical insights into their chemical composition, formation, and evolution history. Ultra-hot Jupiters serve...
  • Publication
    Thermal Instability in a Cooling and Expanding Medium Including Self-Gravity and Conduction
    A systematic study of the linear thermal stability of a medium subject to cooling, self-gravity, and thermal conduction is carried out for the case when the...
  • Publication
    Thermodynamic fluctuations in solar photospheric three-dimensional convection simulations and observations
    Not Available
  • Publication
    Thermodynamic fluctuations in solar photospheric three-dimensional convection simulations and observations
    Context. Numerical three-dimensional (3D) radiative (magneto-)hydrodynamical [(M)HD] simulations of solar convection are nowadays used to understand the...
  • Publication
    Thin coronal jets and plasmoid-mediated reconnection: Insights from Solar Orbiter observations and Bifrost simulations
    Context. Coronal jets are ubiquitous, collimated million-degree ejections that contribute to the energy and mass supply of the upper solar atmosphere and the...
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    Three-dimensional modeling of chromospheric spectral lines in a simulated active region
    Context. Because of the complex physics that governs the formation of chromospheric lines, interpretation of solar chromospheric observations is difficult. The...
  • Publication
    Three-dimensional simulations of solar magneto-convection including effects of partial ionization
    In recent decades, REALISTIC three-dimensional radiative-magnetohydrodynamic simulations have become the dominant theoretical tool for understanding the complex...
  • Publication
    Three-dimensional Spectral Classification of Low-Metallicity Stars Using Artificial Neural Networks
    We explore the application of artificial neural networks (ANNs) for the estimation of atmospheric parameters (Teff, logg, and [Fe/H]) for Galactic F- and G-type...
  • Publication
    Three-dimensional structure of a sunspot light bridge
    Context. Active regions are the most prominent manifestations of solar magnetic fields; their generation and dissipation are fundamental problems in solar...